Escape fractions of Lyα vs. LyC. The plots here show progressively brighter sample selection for all galaxies (top left) and galaxies with erg (top right), erg (bottom left), and erg (bottom right). In each plot we include the and of observed LCEs from Table 1 (blue points) with their error bars. The observed LCEs are all bright in Lyα, with erg s⁻¹. For a few galaxies, the observed is an upper limit; these galaxies are marked by blue arrows. The dashed black line shows the y = x, or equality, line. The dashed orange line in the bottom-right plot shows a linear fit of the simulated galaxies, which yields a slope of 1.02. This plot shows that if we include all galaxies, including very faint ones, and are very scattered and not correlated, but as we restrict our sample to progressively brighter LAEs, a correlation emerges. Bottom-right panel: simulated galaxies are in the same luminosity range as the observed ones (> 10⁴¹ erg s⁻¹), and the two groups show similar correlations.